AT2025ulz and S250818k: Zooming in with the Hubble Space Telescope
AT2025ulz is an optical/near-infrared transient discovered during follow-up of the candidate gravitational wave (GW) event S250818k. Its young age (≲1 day), rapid decline, and strong color evolution over the first 48 hr classify it as a potential kilonova candidate. In this work, we present the results of our observing campaign, carried out with
Yang, Yu-Han et al.
Fecha de publicación:
1
2026